Moving mountains and white spots of Ceres
Alex Soumbatov Gur

TL;DR
This paper proposes a new geological process involving explosive conical cleavage and crustal stresses to explain bright spots, unusual mountains, and craters observed on Ceres, supported by analysis of planetary relief features.
Contribution
It introduces a novel mechanism of explosive ejective orogenesis driven by crustal stresses, explaining planetary surface features like bright spots and mountains.
Findings
Explosive conical cleavage can eject mountains upside down.
Crustal stresses cause crack expansion leading to relief features.
Bright substances are associated with ejective orogenesis.
Abstract
Among surprising results of NASA's Dawn spacecraft mission at dwarf planet Ceres are enigmatic bright spots inside Occator crater and a lone tall pyramid mountain. Here we explain the appearance of such spots, weird mountains, and concomitant craters on celestial bodies. The phenomenon is as follows. A mountain is ejected rotated out of mechanically stressed crust as a result of explosive conical cleavage all over its buried surface. Then the mountain lands upside down i.e. summit up. It may save its integrity or split into parts to form mountains of smaller sizes and/or block debris. The process is a volcanic caldera formation regime. We infer that it is the result of crack expansion and fracture of planetary crust due to inherent stresses. We scrutinize the processes' phenomenology on examples of Ceres' relief features. Pile-ups of bright substances are also synthesized in the course…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Stellar, planetary, and galactic studies
